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Neutrino Oscillations as a Probe of Light Scalar Dark Matter

Asher Berlin
Phys. Rev. Lett. 117, 231801 – Published 30 November 2016

Abstract

We consider a class of models involving interactions between ultralight scalar dark matter and standard model neutrinos. Such couplings modify the neutrino mass splittings and mixing angles to include additional components that vary in time periodically with a frequency and amplitude set by the mass and energy density of the dark matter. Null results from recent searches for anomalous periodicities in the solar neutrino flux strongly constrain the dark matter-neutrino coupling to be orders of magnitude below current and projected limits derived from observations of the cosmic microwave background.

  • Figure
  • Received 7 August 2016

DOI:https://doi.org/10.1103/PhysRevLett.117.231801

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Asher Berlin

  • Department of Physics, Enrico Fermi Institute, University of Chicago, Chicago 60637-1433, Illinois, USA

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Issue

Vol. 117, Iss. 23 — 2 December 2016

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Images

  • Figure 1
    Figure 1

    Regions in the mϕgϕ plane that are ruled out by either Planck measurements of the CMB or searches for time-varying signals in the solar neutrino data of Super-K and SNO. We also show the projected reach of the LENA liquid scintillator neutrino experiment. On the top axis, for each value of mϕ we display the corresponding period (in days) of the modulation imprinted on the solar neutrino flux τϕ2π/mϕ. In the gray shaded region, dark matter lighter than 1021eV is in slight tension with observations of the Lyman-α forest. Current searches for anomalous periodicities in the solar neutrino data can probe DM-neutrino couplings that are orders of magnitude below limits derived from cosmological observations.

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